| Introduction | |
| The Case for the Relativistic Hot Big Bang Cosmology | p. 3 |
| The Evolution of the Universe | p. 11 |
| An Unbound Universe? | p. 18 |
| The Big Bang Strikes Back | p. 29 |
| Big Bang Nucleosynthesis: The Standard Model and Alternatives | p. 35 |
| Primordial Nucleosynthesis Redux | p. 43 |
| On the Origin of Light Elements | p. 65 |
| The Origin of Deuterium | p. 87 |
| What Can Deuterium Tell Us? | p. 93 |
| Constraints on the Density of Baryons in the Universe | p. 100 |
| Contamination of Primordial Helium in Galaxies | p. 115 |
| Destruction of [superscript 3]He in Stars | p. 126 |
| Limits to the Primordial Helium Abundance in the Baryon-Inhomogeneous Big Bang | p. 130 |
| Lithium Probes the Universe | p. 137 |
| Population II [superscript 6]Li as a Probe of Nucleosynthesis and Stellar Structure and Evolution | p. 138 |
| Main Sequence Mass Loss and the Lithium Dip | p. 142 |
| Effects of Convective Overshoot on Lithium Depletion in Main-Sequence Stars | p. 146 |
| Mass Loss and a Possible Population II Lithium Dip | p. 153 |
| Cosmological Limits to the Number of Massive Leptons | p. 159 |
| Cosmology and the Neutron Lifetime | p. 162 |
| On the Relation of the Cosmological Constraints on Neutrino Flavors to the Width of the Z[superscript 0] | p. 167 |
| Particle Accelerators Test Cosmological Theory | p. 172 |
| Cosmological Constraints on Superweak Particles | p. 181 |
| Limits from Supernovae on Neutrino Radiative Lifetimes | p. 185 |
| Updated Constraints on Axions from SN1987A | p. 188 |
| Astrophysical and Cosmological Constraints to Neutrino Properties | p. 194 |
| Some Astrophysical Consequences of the Existence of a Heavy Stable Neutral Lepton | p. 233 |
| General Cosmological Constraints on the Masses of Stable Neutrinos and Other "Inos" | p. 250 |
| Constraints from Primordial Nucleosynthesis on the Mass of the [tau] Neutrino | p. 272 |
| Astrophysical Constraints on the Couplings of Axions, Majorons, and Familons | p. 276 |
| The Origin of Baryons in the Universe | p. 285 |
| Cosmology and Elementary-Particle Physics | p. 287 |
| The Cosmology/Particle Physics Interface | p. 295 |
| Leptonic and Hadronic Mass Scales - A Cosmic Connection? | p. 324 |
| Spontaneous Generation of Density Perturbations in the Early Universe | p. 333 |
| Quark-Hadron and Chiral Transitions and Their Relation to the Early Universe | p. 336 |
| The Quark-Hadron Transition in the Early Universe | p. 348 |
| Big Bang Nucleosynthesis and the Quark-Hadron Transition | p. 363 |
| Production of Lithium, Beryllium, and Boron From Baryon Inhomogeneous Primordial Nucleosynthesis | p. 368 |
| Recent Advances in Cosmology | p. 379 |
| The Phenomenological Status of Late Time Phase Transition Models after Cosmic Background Radiation Anisotropy Measurements | p. 392 |
| Fractals and Cosmological Large-Scale Structure | p. 399 |
| Are Galaxies More Strongly Correlated Than Clusters? | p. 402 |
| Cosmological Structure Formation from Soft Topological Defects | p. 407 |
| Testing for the Gaussian Nature of Cosmological Density Perturbations through the Three-Point Temperature Correlation Function | p. 422 |
| Strings and the Origins of Galaxies | p. 426 |
| Can "Warm" Particles Provide the Missing Mass in Dwarf Galaxies? | p. 428 |
| Galaxy and Structure Formation with Hot Dark Matter and Cosmic Strings | p. 435 |
| Relic Neutrinos and the Density of the Universe | p. 439 |
| Dark Matter and the Origin of Cosmic Structure | p. 446 |
| The Age of the Universe: Concordance | p. 455 |
| Nucleochronologies and the Mean Age of the Elements | p. 474 |
| r-Process Production Ratios of Chronologic Importance | p. 487 |
| Urban High Energy Cosmic Ray Neutrinos | p. 495 |
| OB Associations and the Nonuniversality of the Cosmic Abundances: Implications for Cosmic Rays and Meteorites | p. 501 |
| Implications of the Ultrahigh-Energy Cosmic-Ray Spectrum Observed by the Fly's Eye Detector | p. 508 |
| Beryllium and Boron Constraints on an Early Galactic Bright Phase | p. 512 |
| Grand Unified Theories, Topological Defects and Ultrahigh-Energy Cosmic Rays | p. 520 |
| Photon/Proton Ratio as a Diagnostic Tool for Topological Defects as the Sources of Extremely High-Energy Cosmic Rays | p. 524 |
| On the Origin of Highest Energy Cosmic Rays | p. 529 |
| High Energy Neutrino Astronomy | p. 543 |
| Origin of Cosmic Rays, Atomic Nuclei and Pulsars in Explosions of Massive Stars | p. 549 |
| Neutral Currents and Supernovas | p. 554 |
| On the Conditions Required for the r-Process | p. 558 |
| Neutrino Damping of Nonradial Pulsations in Gravitational Collapse | p. 570 |
| Supernovae, Grains and the Formation of the Solar System | p. 577 |
| Neutrinos From Gravitational Collapse | p. 580 |
| Supernova 1987A: 18 Months Later | p. 599 |
| The Great Supernova of 1987 | p. 623 |
| Supernova Neutrinos | p. 628 |
| Did a Supernova Trigger the Formation of the Solar System? | p. 632 |
| Protogalactic Mergers and Cosmochronology | p. 647 |
| On the Origin and Evolution of s-Process Elements | p. 655 |
| Black-Hole-Neutron-Star Collisions | p. 663 |
| Magneto-hydrodynamics Jets, Pulsar Formation and SN1987a | p. 666 |
| Antineutrino Astronomy and Geophysics | p. 674 |
| Nucleosynthesis, Neutrino Bursts and [gamma]-rays From Coalescing Neutron Stars | p. 682 |
| The Need for New Neutrino Physics or a Cooler Sun in the Solar Neutrino Problem | p. 687 |
| Monte Carlo Exploration of Mikheyev-Smirnov-Wolfenstein Solutions to the Solar Neutrino Problem | p. 701 |
| Neutrinos From a Standard Solar Model | p. 705 |
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